Predicting emission line fluxes and number counts of distant galaxies for cosmological surveys


Abstract in English

We estimate the number counts of line emitters at high redshift and their evolution with cosmic time based on a combination of photometry and spectroscopy. We predict the H$alpha$, H$beta$, [OII], and [OIII] line fluxes for more than $35,000$ galaxies down to stellar masses of $sim10^9$ $M_{odot}$ in the COSMOS and GOODS-S fields, applying standard

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